New extended radio sources from the NVSS

Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio...
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Autor*in:	Amirkhanyan, V. R. [verfasserIn] Afanasiev, V. L. Moiseev, A. V.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	galaxies: general radio continuum: galaxies

Anmerkung:	© Pleiades Publishing, Ltd. 2015

Übergeordnetes Werk:	Enthalten in: Astrophysical bulletin - Moscow : MAIK Nauka/Interperiodica Publ., 2007, 70(2015), 1 vom: Jan., Seite 45-50
Übergeordnetes Werk:	volume:70 ; year:2015 ; number:1 ; month:01 ; pages:45-50

Links:	Volltext

DOI / URN:	10.1134/S1990341315010058

Katalog-ID:	SPR022821287

Internformat


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520			\|a Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources.
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700	1		\|a Afanasiev, V. L. \|4 aut
700	1		\|a Moiseev, A. V. \|4 aut
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912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_120
912			\|a GBV_ILN_138
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_171
912			\|a GBV_ILN_187
912			\|a GBV_ILN_213
912			\|a GBV_ILN_224
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912			\|a GBV_ILN_250
912			\|a GBV_ILN_281
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_636
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2001
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2004
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2010
912			\|a GBV_ILN_2011
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2015
912			\|a GBV_ILN_2020
912			\|a GBV_ILN_2021
912			\|a GBV_ILN_2025
912			\|a GBV_ILN_2026
912			\|a GBV_ILN_2027
912			\|a GBV_ILN_2031
912			\|a GBV_ILN_2034
912			\|a GBV_ILN_2037
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912			\|a GBV_ILN_2044
912			\|a GBV_ILN_2048
912			\|a GBV_ILN_2049
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912			\|a GBV_ILN_2336
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912			\|a GBV_ILN_2522
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912			\|a GBV_ILN_4037
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952			\|d 70 \|j 2015 \|e 1 \|c 01 \|h 45-50

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publishDate	2015
allfields	10.1134/S1990341315010058 doi (DE-627)SPR022821287 (SPR)S1990341315010058-e DE-627 ger DE-627 rakwb eng Amirkhanyan, V. R. verfasserin aut New extended radio sources from the NVSS 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. galaxies: general (dpeaa)DE-He213 radio continuum: galaxies (dpeaa)DE-He213 Afanasiev, V. L. aut Moiseev, A. V. aut Enthalten in Astrophysical bulletin Moscow : MAIK Nauka/Interperiodica Publ., 2007 70(2015), 1 vom: Jan., Seite 45-50 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:70 year:2015 number:1 month:01 pages:45-50 https://dx.doi.org/10.1134/S1990341315010058 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 70 2015 1 01 45-50
spelling	10.1134/S1990341315010058 doi (DE-627)SPR022821287 (SPR)S1990341315010058-e DE-627 ger DE-627 rakwb eng Amirkhanyan, V. R. verfasserin aut New extended radio sources from the NVSS 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. galaxies: general (dpeaa)DE-He213 radio continuum: galaxies (dpeaa)DE-He213 Afanasiev, V. L. aut Moiseev, A. V. aut Enthalten in Astrophysical bulletin Moscow : MAIK Nauka/Interperiodica Publ., 2007 70(2015), 1 vom: Jan., Seite 45-50 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:70 year:2015 number:1 month:01 pages:45-50 https://dx.doi.org/10.1134/S1990341315010058 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 70 2015 1 01 45-50
allfields_unstemmed	10.1134/S1990341315010058 doi (DE-627)SPR022821287 (SPR)S1990341315010058-e DE-627 ger DE-627 rakwb eng Amirkhanyan, V. R. verfasserin aut New extended radio sources from the NVSS 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. galaxies: general (dpeaa)DE-He213 radio continuum: galaxies (dpeaa)DE-He213 Afanasiev, V. L. aut Moiseev, A. V. aut Enthalten in Astrophysical bulletin Moscow : MAIK Nauka/Interperiodica Publ., 2007 70(2015), 1 vom: Jan., Seite 45-50 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:70 year:2015 number:1 month:01 pages:45-50 https://dx.doi.org/10.1134/S1990341315010058 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 70 2015 1 01 45-50
allfieldsGer	10.1134/S1990341315010058 doi (DE-627)SPR022821287 (SPR)S1990341315010058-e DE-627 ger DE-627 rakwb eng Amirkhanyan, V. R. verfasserin aut New extended radio sources from the NVSS 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. galaxies: general (dpeaa)DE-He213 radio continuum: galaxies (dpeaa)DE-He213 Afanasiev, V. L. aut Moiseev, A. V. aut Enthalten in Astrophysical bulletin Moscow : MAIK Nauka/Interperiodica Publ., 2007 70(2015), 1 vom: Jan., Seite 45-50 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:70 year:2015 number:1 month:01 pages:45-50 https://dx.doi.org/10.1134/S1990341315010058 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 70 2015 1 01 45-50
allfieldsSound	10.1134/S1990341315010058 doi (DE-627)SPR022821287 (SPR)S1990341315010058-e DE-627 ger DE-627 rakwb eng Amirkhanyan, V. R. verfasserin aut New extended radio sources from the NVSS 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. galaxies: general (dpeaa)DE-He213 radio continuum: galaxies (dpeaa)DE-He213 Afanasiev, V. L. aut Moiseev, A. V. aut Enthalten in Astrophysical bulletin Moscow : MAIK Nauka/Interperiodica Publ., 2007 70(2015), 1 vom: Jan., Seite 45-50 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:70 year:2015 number:1 month:01 pages:45-50 https://dx.doi.org/10.1134/S1990341315010058 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 70 2015 1 01 45-50
language	English
source	Enthalten in Astrophysical bulletin 70(2015), 1 vom: Jan., Seite 45-50 volume:70 year:2015 number:1 month:01 pages:45-50
sourceStr	Enthalten in Astrophysical bulletin 70(2015), 1 vom: Jan., Seite 45-50 volume:70 year:2015 number:1 month:01 pages:45-50
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	galaxies: general radio continuum: galaxies
isfreeaccess_bool	false
container_title	Astrophysical bulletin
authorswithroles_txt_mv	Amirkhanyan, V. R. @@aut@@ Afanasiev, V. L. @@aut@@ Moiseev, A. V. @@aut@@
publishDateDaySort_date	2015-01-01T00:00:00Z
hierarchy_top_id	546895565
id	SPR022821287
language_de	englisch
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author	Amirkhanyan, V. R.
spellingShingle	Amirkhanyan, V. R. misc galaxies: general misc radio continuum: galaxies New extended radio sources from the NVSS
authorStr	Amirkhanyan, V. R.
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topic_title	New extended radio sources from the NVSS galaxies: general (dpeaa)DE-He213 radio continuum: galaxies (dpeaa)DE-He213
topic	misc galaxies: general misc radio continuum: galaxies
topic_unstemmed	misc galaxies: general misc radio continuum: galaxies
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format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
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title	New extended radio sources from the NVSS
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title_full	New extended radio sources from the NVSS
author_sort	Amirkhanyan, V. R.
journal	Astrophysical bulletin
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author_browse	Amirkhanyan, V. R. Afanasiev, V. L. Moiseev, A. V.
container_volume	70
format_se	Elektronische Aufsätze
author-letter	Amirkhanyan, V. R.
doi_str_mv	10.1134/S1990341315010058
title_sort	new extended radio sources from the nvss
title_auth	New extended radio sources from the NVSS
abstract	Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. © Pleiades Publishing, Ltd. 2015
abstractGer	Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. © Pleiades Publishing, Ltd. 2015
abstract_unstemmed	Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources. © Pleiades Publishing, Ltd. 2015
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container_issue	1
title_short	New extended radio sources from the NVSS
url	https://dx.doi.org/10.1134/S1990341315010058
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author2	Afanasiev, V. L. Moiseev, A. V.
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up_date	2024-07-03T15:04:45.848Z
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R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">New extended radio sources from the NVSS</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Pleiades Publishing, Ltd. 2015</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract We report the results of the spectroscopic observations carried out at the SAO RAS 6-m telescope for the optical components of nine new extended radio sources found in the NVSS catalog. The measured redshifts of the host galaxies lie in the range of z = 0.1–0.4. Physical sizes of the radio sources were calculated within the standard cosmological model. The two most extended objects, 0003+1512 and 0422+0351, reach sizes of 2.1 Mpc and 4.0 Mpc respectively. This is close to the maximum size of known radio sources.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">galaxies: general</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">radio continuum: galaxies</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Afanasiev, V. L.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Moiseev, A. 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